Difference: SUSYCrossSections (1 vs. 42)

Revision 422019-08-09 - AlexanderMann

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SUSY Cross Sections for 7 TeV pp Collisions

Abstract

We summarise the status of the cross section predictions for various supersymmetric processes in pp collisions at sqrt(s)=7 TeV. This document is based on the agreement between the ATLAS and CMS collaborations, as well as with the LPCC SUSY cross section working group. Calculations including the resummation of soft gluon emission at the next-to-leading logarithmic accuracy are used whenever available. In all other cases we rely on the next-to-leading order in the strong coupling constant. These cross sections and their uncertainties are provided for various scale and PDF choices.

Cross sections for various subprocesses

Important notice: ATLAS and CMS used the same CMSSM tanbeta grid but the program performing the Renormalisation Group Equations is different (ATLAS is using ISAJET whereas CMS is using SOFTSUSY). These different programs lead to differences in mass at the 7 TeV scale. In particular, for the same starting m0 and m1/2 combination, the sparticle masses used in ATLAS are usually slightly higher than the ones used in CMS case. This effect has two effects which partially cancel each other: on the one hand, CMS cross sections are higher than those of ATLAS but, on the other hand, ATLAS scenarios tend to have slightly harder jet pT spectrum, leading to a slightly higher acceptance in most of the analyses. The SUSY Working Groups of the two collaborations agreed to use the same generator for analyses using 8 TeV centre-of-mass energy.

Documentation

SUSY Cross Sections for 8 TeV pp Collisions

Abstract

We summarise the status of the cross section predictions for various supersymmetric processes in pp collisions at sqrt(s)=8 TeV. This document is based on the agreement between the ATLAS and CMS collaborations, as well as with the LPCC SUSY cross section working group. Calculations including the resummation of soft gluon emission at the next-to-leading logarithmic accuracy are used whenever available. In all other cases we rely on the next-to-leading order in the strong coupling constant. These cross sections and their uncertainties are provided for various scale and PDF choices.

Documentation

Cross sections for various subprocesses

The cross sections for the associated production of mass degenerate chargino1 and neutralino2 calculated by ATLAS and by CMS differ due to the non-zero higgsino component assumed in the ATLAS model.
 

SUSY Cross Sections for 13, 14, 33 and 100 TeV pp Collisions

Abstract

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Cross-section plots

The following plots show the cross-section values from the TWiki pages above:

overview strong weak

The code to make these plots can be found on github.

 

Cross sections for various subprocesses - 14 TeV

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  Reference: Squark and gluino production cross sections in pp collisions at \sqrt(s) = 13, 14, 33 and 100 TeV, C. Borschensky, M. Kramer, A. Kulesza, M. Mangano, S. Padhi, T. Plehn, X. Portell, arXiv:1407.5066, Published in Eur.Phys.J. C74 (2014) 12
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SUSY Cross Sections for 7 TeV pp Collisions

Abstract

We summarise the status of the cross section predictions for various supersymmetric processes in pp collisions at sqrt(s)=7 TeV. This document is based on the agreement between the ATLAS and CMS collaborations, as well as with the LPCC SUSY cross section working group. Calculations including the resummation of soft gluon emission at the next-to-leading logarithmic accuracy are used whenever available. In all other cases we rely on the next-to-leading order in the strong coupling constant. These cross sections and their uncertainties are provided for various scale and PDF choices.

Cross sections for various subprocesses

Important notice: ATLAS and CMS used the same CMSSM tanbeta grid but the program performing the Renormalisation Group Equations is different (ATLAS is using ISAJET whereas CMS is using SOFTSUSY). These different programs lead to differences in mass at the 7 TeV scale. In particular, for the same starting m0 and m1/2 combination, the sparticle masses used in ATLAS are usually slightly higher than the ones used in CMS case. This effect has two effects which partially cancel each other: on the one hand, CMS cross sections are higher than those of ATLAS but, on the other hand, ATLAS scenarios tend to have slightly harder jet pT spectrum, leading to a slightly higher acceptance in most of the analyses. The SUSY Working Groups of the two collaborations agreed to use the same generator for analyses using 8 TeV centre-of-mass energy.

Documentation

SUSY Cross Sections for 8 TeV pp Collisions

Abstract

We summarise the status of the cross section predictions for various supersymmetric processes in pp collisions at sqrt(s)=8 TeV. This document is based on the agreement between the ATLAS and CMS collaborations, as well as with the LPCC SUSY cross section working group. Calculations including the resummation of soft gluon emission at the next-to-leading logarithmic accuracy are used whenever available. In all other cases we rely on the next-to-leading order in the strong coupling constant. These cross sections and their uncertainties are provided for various scale and PDF choices.

Documentation

Cross sections for various subprocesses

The cross sections for the associated production of mass degenerate chargino1 and neutralino2 calculated by ATLAS and by CMS differ due to the non-zero higgsino component assumed in the ATLAS model.
 
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Revision 402019-07-12 - AlexanderMann

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Contributors: Christoph Borschensky, Zoltan Gecse, Michael Kraemer, Robin van der Leeuw, Anna Kulesza, Michelangelo Mangano, Sanjay Padhi, Tilman Plehn, Xavier Portell, Sezen Sekmen

Mailing list: lhc-susy-cross-section-wg@cernNOSPAMch, archive.

>
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  • Contributors: Christoph Borschensky, Zoltan Gecse, Michael Kraemer, Robin van der Leeuw, Anna Kulesza, Michelangelo Mangano, Sanjay Padhi, Tilman Plehn, Xavier Portell, Sezen Sekmen
  • Mailing list: lhc-susy-cross-section-wg@cernNOSPAMch, archive.
  • The cross-section values from these TWiki pages are available in JSON format in this public git repository on github. (So far it only contains the 13 TeV cross sections.)
 
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Overview

gluino_xsec.png squark_xsec.png stop_xsec.png

Reference: Squark and gluino production cross sections in pp collisions at \sqrt(s) = 13, 14, 33 and 100 TeV, C. Borschensky, M. Kramer, A. Kulesza, M. Mangano, S. Padhi, T. Plehn, X. Portell, arXiv:1407.5066, Published in Eur.Phys.J. C74 (2014) 12

 

SUSY Cross Sections for 7 TeV pp Collisions

Abstract

We summarise the status of the cross section predictions for various supersymmetric processes in pp collisions at sqrt(s)=7 TeV. This document is based on the agreement between the ATLAS and CMS
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collaborations, as well as with the LPCC SUSY cross section working group. Calculations including
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collaborations, as well as with the LPCC SUSY cross section working group. Calculations including
 the resummation of soft gluon emission at the next-to-leading logarithmic accuracy are used whenever available. In all other cases we rely on the next-to-leading order in the strong coupling constant. These cross sections and their uncertainties are provided for various scale and PDF choices.
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  We summarise the status of the cross section predictions for various supersymmetric processes in pp collisions at sqrt(s)=8 TeV. This document is based on the agreement between the ATLAS and CMS
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collaborations, as well as with the LPCC SUSY cross section working group. Calculations including
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collaborations, as well as with the LPCC SUSY cross section working group. Calculations including
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  We summarise the status of the cross section predictions for various supersymmetric processes in pp collisions at sqrt(s)=13, 14, 33 and 100 TeV. This document is based on the agreement between the ATLAS and CMS
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collaborations, as well as with the LPCC SUSY cross section working group. Calculations including
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collaborations, as well as with the LPCC SUSY cross section working group. Calculations including
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Overview (Strong Production Only)

gluino_xsec.png squark_xsec.png stop_xsec.png

Reference: Squark and gluino production cross sections in pp collisions at \sqrt(s) = 13, 14, 33 and 100 TeV, C. Borschensky, M. Kramer, A. Kulesza, M. Mangano, S. Padhi, T. Plehn, X. Portell, arXiv:1407.5066, Published in Eur.Phys.J. C74 (2014) 12

 
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Revision 392019-05-06 - AlexanderMann

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Documentation

Colored Sector
  • NLO + NLL Tool for 13, 14, 33 and 100 TeV cross sections.
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  Electroweak Sector
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*NLO+NLL threshold resummed results
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NLO+NLL threshold resummed results.
 
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For Sleptons production:
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For slepton production:
 
  • G. Bozzi, B. Fuks, and M. Klasen, Nucl. Phys. B 777, 157 (2007)
  • B. Fuks, M. Klasen, D. R. Lamprea, and M. Rothering, Eur. Phys. J. C 73, 2480 (2013)
  • B. Fuks, M. Klasen, D. R. Lamprea and M. Rothering, JHEP01(2014)168 
  • J. Fiaschi and M. Klasen, JHEP 1803 (2018) 094
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For Gauginos production:
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For gaugino production:
 
  • J. Debove, B. Fuks, and M. Klasen, Nucl. Phys. B 842, 51 (2011)
  • B. Fuks, M. Klasen, D. R. Lamprea, and M. Rothering, JHEP 1210, 081 (2012)
  • B. Fuks, M. Klasen, D. R. Lamprea, and M. Rothering, Eur. Phys. J. C 73, 2480 (2013)

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LHC SUSY Cross Section Working Group

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LHC SUSY Cross Section Working Group

  Contributors: Christoph Borschensky, Zoltan Gecse, Michael Kraemer, Robin van der Leeuw, Anna Kulesza, Michelangelo Mangano, Sanjay Padhi, Tilman Plehn, Xavier Portell, Sezen Sekmen
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  Reference: Squark and gluino production cross sections in pp collisions at \sqrt(s) = 13, 14, 33 and 100 TeV, C. Borschensky, M. Kramer, A. Kulesza, M. Mangano, S. Padhi, T. Plehn, X. Portell, arXiv:1407.5066, Published in Eur.Phys.J. C74 (2014) 12
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SUSY Cross Sections using 7 TeV pp collisions

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SUSY Cross Sections for 7 TeV pp Collisions

 

Abstract

We summarise the status of the cross section predictions for various supersymmetric processes in pp
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 available. In all other cases we rely on the next-to-leading order in the strong coupling constant. These cross sections and their uncertainties are provided for various scale and PDF choices.
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Cross sections for various Sub-process

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Cross sections for various subprocesses

  Important notice: ATLAS and CMS used the same CMSSM tanbeta grid but the program performing the Renormalisation Group Equations is different (ATLAS is using ISAJET whereas CMS is using SOFTSUSY). These different programs lead to differences in mass at the 7 TeV scale. In particular, for the same starting m0 and m1/2 combination, the sparticle masses used in ATLAS are usually slightly higher than the ones used in CMS case. This effect has two effects which partially cancel each other: on the one hand, CMS cross sections are higher than those of ATLAS but, on the other hand, ATLAS scenarios tend to have slightly harder jet pT spectrum, leading to a slightly higher acceptance in most of the analyses. The SUSY Working Groups of the two collaborations agreed to use the same generator for analyses using 8 TeV centre-of-mass energy.
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SUSY Cross Sections using 8 TeV pp collisions

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SUSY Cross Sections for 8 TeV pp Collisions

 

Abstract

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Cross sections for various Sub-process

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Cross sections for various subprocesses

 
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SUSY Cross Sections using 13, 14, 33 and 100 TeV pp collisions

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SUSY Cross Sections for 13, 14, 33 and 100 TeV pp Collisions

 

Abstract

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  • B. Fuks, M. Klasen, D. R. Lamprea, and M. Rothering, Eur. Phys. J. C 73, 2480 (2013)
  • J. Fiaschi and M. Klasen, Phys.Rev. D98 (2018) 055014
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Cross sections for various Sub-process - 13 TeV

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Cross sections for various subprocesses - 13 TeV

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  Electroweak Sector
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Cross sections for various Sub-process - 14 TeV

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Cross sections for various subprocesses - 14 TeV

 
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Cross sections for various Sub-process - 33 TeV

Cross sections for various Sub-process - 100 TeV

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Cross sections for various subprocesses - 33 TeV

Cross sections for various subprocesses - 100 TeV

 

-- SanjayPadhi - 03-Jun-2012

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 cross sections and their uncertainties are provided for various scale and PDF choices.

Documentation

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Colored Sector
 
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Electroweak Sector

*NLO+NLL threshold resummed results

For Sleptons production:

  • G. Bozzi, B. Fuks, and M. Klasen, Nucl. Phys. B 777, 157 (2007)
  • B. Fuks, M. Klasen, D. R. Lamprea, and M. Rothering, Eur. Phys. J. C 73, 2480 (2013)
  • B. Fuks, M. Klasen, D. R. Lamprea and M. Rothering, JHEP01(2014)168 
  • J. Fiaschi and M. Klasen, JHEP 1803 (2018) 094

For Gauginos production:

  • J. Debove, B. Fuks, and M. Klasen, Nucl. Phys. B 842, 51 (2011)
  • B. Fuks, M. Klasen, D. R. Lamprea, and M. Rothering, JHEP 1210, 081 (2012)
  • B. Fuks, M. Klasen, D. R. Lamprea, and M. Rothering, Eur. Phys. J. C 73, 2480 (2013)
  • J. Fiaschi and M. Klasen, Phys.Rev. D98 (2018) 055014
 

Cross sections for various Sub-process - 13 TeV

Colored Sector

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Cross sections for various Sub-process - 13 TeV

Colored Sector

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  Electroweak Sector
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Cross sections for various Sub-process - 33 TeV

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Cross sections for various Sub-process - 33 TeV

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 The cross sections for the associated production of mass degenerate chargino1 and neutralino2 calculated by ATLAS and by CMS differ due to the non-zero higgsino component assumed in the ATLAS model.
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SUSY Cross Sections using 13, 14, 33 and 100 TeV pp collisions

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Cross sections for various Sub-process - 13 TeV

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Colored Sector
 
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Electroweak Sector
 

Cross sections for various Sub-process - 14 TeV

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Documentation

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  • NLO + NLL Tool for 13, 14, 33 and 100 TeV cross sections.
 

Cross sections for various Sub-process - 13 TeV

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 squark_xsec.png stop_xsec.png
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Reference: Squark and gluino production cross sections in pp collisions at \sqrt(s) = 13, 14, 33 and 100 TeV, C. Borschensky, M. Kramer, A. Kulesza, M. Mangano, S. Padhi, T. Plehn, X. Portell, arXiv:1407.5066, Published in Eur.Phys.J. C74 (2014) 12
 

SUSY Cross Sections using 7 TeV pp collisions

Abstract

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Documentation

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Cross sections for various Sub-process - 13 TeV

Revision 282014-09-02 - ZoltanGecse

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Contributors: Christoph Borschensky, Zoltan Gecse, Michael Kraemer, Robin van der Leeuw, Anna Kulesza, Michelangelo Mangano, Sanjay Padhi, Tilman Plehn, Xavier Portell, Sezen Sekmen

Mailing list: lhc-susy-cross-section-wg@cernNOSPAMch, archive.

 

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Contributors: Christoph Borschensky, Zoltan Gecse, Anna Kulesza, Michael Kraemer, Michelangelo Mangano, Sanjay Padhi, Tilman Plehn, Sezen Sekmen
 

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Revision 252014-07-24 - SanjayPadhi

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Contributors: Christoph Borschensky, Anna Kulesza, Michael Kraemer, Robin van der Leeuw, Michelangelo Mangano, Sanjay Padhi, Tilman Plehn, Xavier Portell, Sezen Sekmen
 
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 -- XavierPortell - 07-Jun-2012 -- FrankWuerthwein - 30-Jan-2013
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Revision 242014-07-24 - SanjayPadhi

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Abstract

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 -- XavierPortell - 07-Jun-2012 -- FrankWuerthwein - 30-Jan-2013
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META FILEATTACHMENT attachment="sqsq_decoupled7TeV.txt" attr="h" comment="" date="1339497191" name="sqsq_decoupled7TeV.txt" path="sqsq_decoupled7TeV.txt" size="16400" user="spadhi" version="1"
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Revision 222014-07-21 - SanjayPadhi

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SUSY Cross Sections using 13, 14, 33 and 100 TeV pp collisions

 

Abstract

We summarise the status of the cross section predictions for various supersymmetric processes in pp

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collisions at sqrt(s)=13 TeV. This document is based on the agreement between the ATLAS and CMS
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collisions at sqrt(s)=13, 14, 33 and 100 TeV. This document is based on the agreement between the ATLAS and CMS
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Cross sections for various Sub-process - 33 TeV

Cross sections for various Sub-process - 100 TeV

 -- SanjayPadhi - 03-Jun-2012 -- XavierPortell - 07-Jun-2012 -- FrankWuerthwein - 30-Jan-2013

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 available. In all other cases we rely on the next-to-leading order in the strong coupling constant. These cross sections and their uncertainties are provided for various scale and PDF choices.
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 available. In all other cases we rely on the next-to-leading order in the strong coupling constant. These cross sections and their uncertainties are provided for various scale and PDF choices.
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SUSY Cross Sections using 13 TeV pp collisions

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We summarise the status of the cross section predictions for various supersymmetric processes in pp collisions at sqrt(s)=13 TeV. This document is based on the agreement between the ATLAS and CMS collaborations, as well as with the LPCC SUSY cross section working group. Calculations including the resummation of soft gluon emission at the next-to-leading logarithmic accuracy are used whenever available. In all other cases we rely on the next-to-leading order in the strong coupling constant. These cross sections and their uncertainties are provided for various scale and PDF choices.

Cross sections for various Sub-process

  -- SanjayPadhi - 03-Jun-2012 -- XavierPortell - 07-Jun-2012

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The cross sections for the associated production of mass degenerate chargino1 and neutralino2 calculated by ATLAS and by CMS differ due to the non-zero higgsino component assumed in the ATLAS model.
  -- SanjayPadhi - 03-Jun-2012 -- XavierPortell - 07-Jun-2012

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Abstract

 We summarise the status of the cross section predictions for various supersymmetric processes in pp collisions at sqrt(s)=8 TeV. This document is based on the agreement between the ATLAS and CMS collaborations, as well as with the LPCC SUSY cross section working group. Calculations including
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 available. In all other cases we rely on the next-to-leading order in the strong coupling constant. These cross sections and their uncertainties are provided for various scale and PDF choices.
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 Important notice: ATLAS and CMS used the same CMSSM tanbeta grid but the program performing the Renormalisation Group Equations is different (ATLAS is using ISAJET whereas CMS is using SOFTSUSY). These different programs lead to differences in mass at the 7 TeV scale. In particular, for the same starting m0 and m1/2 combination, the sparticle masses used in ATLAS are usually slightly higher than the ones used in CMS case. This effect has two effects which partially cancel each other: on the one hand, CMS cross sections are higher than those of ATLAS but, on the other hand, ATLAS scenarios tend to have slightly harder jet pT spectrum, leading to a slightly higher acceptance in most of the analyses. The SUSY Working Groups of the two collaborations agreed to use the same generator for analyses using 8 TeV centre-of-mass energy.

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SUSY Cross Sections using 7 TeV pp collisions

 

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We summarise the status of the cross section predictions for various supersymmetric processes in pp
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collisions at sqrt(s)=7 TeV. This document is based on the agreement between the ATLAS and CMS
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collisions at sqrt(s)=7 TeV. This document is based on the agreement between the ATLAS and CMS
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cross sections and their uncertainties are provided for various scale and PDF choices.
 

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Important notice: ATLAS and CMS used the same CMSSM tanbeta grid but the program performing the Renormalisation Group Equations is different (ATLAS is using ISAJET whereas CMS is using SOFTSUSY). These different programs lead to differences in mass at the 7 TeV scale. In particular, for the same starting m0 and m1/2 combination, the sparticle masses used in ATLAS are usually slightly higher than the ones used in CMS case. This effect has two effects which partially cancel each other: on the one hand, CMS cross sections are higher than those of ATLAS but, on the other hand, ATLAS scenarios tend to have slightly harder jet pT spectrum, leading to a slightly higher acceptance in most of the analyses. The SUSY Working Groups of the two collaborations agreed to use the same generator for analyses using 8 TeV centre-of-mass energy.

 
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collisions at sqrt(s)=8 TeV. This document is based on the agreement between the ATLAS and CMS
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-- SanjayPadhi - 03-Jun-2012 \ No newline at end of file

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Contributors: Anna Kulesza, Michael Kraemer, Robin van der Leeuw, Sanjay Padhi, Tilman Plehn, Xavier Portell
 

Overview

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SUSY Cross Sections using 7 TeV pp collisions

Abstract

We summarise the status of the cross section predictions for various supersymmetric processes in pp collisions at sqrt(s)=7 TeV. This document is based on the agreement between the ATLAS and CMS collaborations, as well as with the LPCC SUSY cross section working group. Calculations including the resummation of soft gluon emission at the next-to-leading logarithmic accuracy are used whenever available. In all other cases we rely on the next-to-leading order in the strong coupling constant. These cross sections and their uncertainties are provided for various scale and PDF choices.

Cross sections for various Sub-process

Documentation

SUSY Cross Sections using 8 TeV pp collisions

We summarise the status of the cross section predictions for various supersymmetric processes in pp collisions at sqrt(s)=8 TeV. This document is based on the agreement between the ATLAS and CMS collaborations, as well as with the LPCC SUSY cross section working group. Calculations including the resummation of soft gluon emission at the next-to-leading logarithmic accuracy are used whenever available. In all other cases we rely on the next-to-leading order in the strong coupling constant. These cross sections and their uncertainties are provided for various scale and PDF choices.

Abstract

Cross sections for various Sub-process

  -- SanjayPadhi - 03-Jun-2012
 
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